There is only a small range of temperatures in which
(i) gas–magnetic field coupling is possible thanks to sufficient ionisation (\(T\gtrsim 1000\)  K; [1]})
and (ii) at the same time the dust has not been evaporated (\(T\lesssim {T_{\textnormal {dest}}}\approx 1500\)  K,
\({T_{\textnormal {dest}}}\)  being the temperature at which the last component of the dust evaporates; [2]}, [3]}).
In other words, in the MagAcc scenario the temperature is usually too high for dust to survive.
Therefore, we will put MagAcc aside for this section.
